Asteroid migration due to the Yarkovsky effect and the distribution of the Eos family
| Autor: | Li Yong Zhou, Yang Bo Xu, Wing-Huen Ip, Christoph Lhotka |
|---|---|
| Rok vydání: | 2020 |
| Předmět: |
Earth and Planetary Astrophysics (astro-ph.EP)
Physics Debris disk 010504 meteorology & atmospheric sciences Mathematical analysis Yarkovsky effect FOS: Physical sciences Equations of motion Perturbation (astronomy) Astronomy and Astrophysics 01 natural sciences Omega Celestial mechanics Space and Planetary Science Asteroid Physics::Space Physics 0103 physical sciences Thermal Astrophysics::Earth and Planetary Astrophysics 010303 astronomy & astrophysics Astrophysics - Earth and Planetary Astrophysics 0105 earth and related environmental sciences |
| Zdroj: | Monthly Notices of the Royal Astronomical Society. 493:1447-1460 |
| ISSN: | 1365-2966 0035-8711 |
| DOI: | 10.1093/mnras/staa352 |
| Popis: | Based on a linearized model of the Yarkovsky effect, we investigate in this paper the dependence of the semimajor axis drift $\Delta a$ of a celestial body on its size, spinning obliquity, initial orbit and thermal parameters on its surface. With appropriate simplification and approximation, we obtain the analytical solutions to the perturbation equations for the motion of asteroids influenced by the Yarkovsky effect, and they are then verified by numerical simulations of the full equations of motion. These solutions present explicitly the dependencies of $\Delta a$ on the thermal and dynamical parameters of the asteroid. With these analytical formulae for $\Delta a$, we investigate the combined seasonal and diurnal Yarkovsky effects. The critical points where the migration direction reverses are calculated and the consequent selective effects according to the size and rotation state of asteroids are discussed. %Solely the Yarkovsky effect is found to be able to produce some ring structure in the aged circumstellar debris disk. Finally, we apply the analytical formulae to calculate the migration of Eos family members. The space distribution of asteroids is well reproduced. Our calculations suggest that statistically the orientations of spin axes of family members satisfy a random-obliquity distribution, and the rotation rate $\omega_{\rm rot}$ of asteroid depends on its size $R$ by $\omega_{\rm rot}\propto R^{-1}$. Comment: 15 pages, 7 figures |
| Databáze: | OpenAIRE |
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